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Streaming Motions toward the Supermassive Black Hole in NGC 1097
Stockholm University, Faculty of Science, Department of Astronomy.
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2006 (English)In: AstrophysicalJournal Letters, Vol. 641, no L25Article in journal (Other (popular science, discussion, etc.)) Published
Abstract [en]

We have used GMOS-IFU and high-resolution HST-ACS observations to map, in unprecedented detail, the gas velocity field and structure within the 0.7 kpc circumnuclear ring of the SBb LINER/Seyfert 1 galaxy NGC 1097. We find clear evidence of radial streaming motions associated with spiral structures leading to the unresolved (<3.5 pc) nucleus, which we interpret as part of the fueling chain by which gas is transported to the nuclear starburst and supermassive black hole.

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2006. Vol. 641, no L25
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URN: urn:nbn:se:su:diva-11536DOI: doi:10.1086/503832OAI: oai:DiVA.org:su-11536DiVA: diva2:178055
Available from: 2008-01-12 Created: 2008-01-12 Last updated: 2011-01-11Bibliographically approved

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